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Related papers: Large scale extragalactic jets powered by very-hig…

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SS433 is a Galactic microquasar with powerful jets, where very-high-energy particles are produced. We study particle acceleration in the jets of SS433 in the light of the recent multi-wavelength data from radio to TeV gamma ray. We first…

High Energy Astrophysical Phenomena · Physics 2020-02-12 Takahiro Sudoh , Yoshiyuki Inoue , Dmitry Khangulyan

The jet charge is an old observable that has proven uniquely useful for discrimination of jets initiated by different flavors of light quarks, for example. In this Letter, we propose an approach to understanding the jet charge by…

High Energy Physics - Phenomenology · Physics 2023-04-27 Zhong-Bo Kang , Andrew J. Larkoski , Jinghong Yang

The innermost parts of powerful jets in active galactic nuclei are surrounded by dense, high-velocity clouds from the broad-line region, which may penetrate into the jet and lead to the formation of a strong shock. Such jet-cloud…

High Energy Astrophysical Phenomena · Physics 2019-03-20 S. del Palacio , V. Bosch-Ramon , G. E. Romero

The power of blazar jets rivals the power that gravity can extract from accreting matter. The mechanism launching and accelerating jets can be considered as the most efficient engine operating in radio--loud sources. It is still a matter of…

Astrophysics · Physics 2009-11-07 G. Ghisellini

The dramatic relativistic jets pointing directly at us in BL Lac objects can be well modelled by bulk motion beaming of synchrotron self-Compton emission powered by a low Eddington fraction accretion flow. Nearly 500 of these AGN are seen…

High Energy Astrophysical Phenomena · Physics 2015-06-17 Emma Gardner , Chris Done

An ejection mechanism of relativistic jets from slim disks is studied. Since the radiation pressure is dominant in the slim disk, radiative energy flow arises along the pressure gradient in the vertical direction. The divergence of the…

High Energy Astrophysical Phenomena · Physics 2024-04-08 Hajime Inoue

The microquasar phenomenon is associated with the production of jets by X-ray binaries and, as such, may be associated with the majority of such systems. In this chapter we briefly outline the associations, definite, probable, possible, and…

Astrophysics · Physics 2015-06-24 Rob Fender , Tom Maccarone

Recent radio observations support a picture for star formation where there is accretion of matter onto a central protostar with the ejection of molecular outflows that can affect the surrounding medium. The impact of a supersonic outflow on…

Astrophysics · Physics 2011-03-10 A. T. Araudo , G. E. Romero , V. Bosch-Ramon , J. M. Paredes

Relativistic stellar jets, produced in binary systems called microquasars, propagate through media with different spatial scales releasing their energy in the form of work and radiation from radio to gamma rays. There are several…

High Energy Astrophysical Phenomena · Physics 2015-06-18 V. Bosch-Ramon

The respective contribution of disk and jet components to the total emission in low luminosity active galactic nuclei (LLAGNs) is an open question. This paper suggests that $\gamma$-rays emitted from electrons accelerated in jets could be a…

High Energy Astrophysical Phenomena · Physics 2015-05-20 Hajime Takami

Striking similarities exist between high energy gamma ray emission from active galactic nuclei (AGN) and gamma ray bursts (GRBs). They suggest that GRBs are generated by inverse Compton scattering from highly relativistic electrons in…

Astrophysics · Physics 2009-10-22 Nir J. Shaviv , Arnon Dar

As powerful gamma-ray engines, blazars -- relativistic plasma jets launched toward Earth from active galactic nuclei -- are manifestly high-energy particle accelerators. Yet, exactly how these jets accelerate particles as well as what they…

High Energy Astrophysical Phenomena · Physics 2025-04-03 John Mehlhaff , Muni Zhou , Vladimir Zhdankin

Solar jets are fast-moving, elongated brightenings related to ejections seen in both images and spectra on all scales from barely visible chromospheric jets to coronal jets extending up to a few solar radii. The largest, most powerful jets…

Solar and Stellar Astrophysics · Physics 2016-12-07 Davina Innes , Radoslav Bucik , Li-Jia Guo , Nariaki Nitta

If the jets of microquasars carry a significant power in the form of relativistic hadrons, then gamma rays and neutrinos can be produced by interactions with matter and photon fields either external or internal to the jet. In this paper I…

Astrophysics · Physics 2009-04-14 Gustavo E. Romero

A sudden release of high energy cosmic rays at the centre of a wind sustaining a spiral magnetic field produces cavities of low density and low magnetic field along the axis. The trajectories of high energy cosmic rays are focussed onto the…

Astrophysics · Physics 2009-11-13 A. R. Bell

Context. Protostellar jets driven by massive protostars are collimated outflows producing high-speed shocks through dense interstellar medium. Fast shocks can accelerate particles up to relativistic energies via diffusive shock…

High Energy Astrophysical Phenomena · Physics 2025-02-04 J. Méndez-Gallego , R. López-Coto , E. de Oña Wilhelmi , R. Fedriani , J. Otero-Santos , Y. Cantürk

Theoretical studies of jet stopping in strongly-coupled QCD-like plasmas have used gauge-gravity duality to find that the maximum stopping distance scales like E^{1/3} for large jet energies E. In recent work studying jets that are created…

High Energy Physics - Theory · Physics 2015-03-17 Peter Arnold , Diana Vaman

Microquasars are binary systems that harbor a normal star and a compact object (black-hole or neutron star), and show relativistic outflows (or jets). The matter that forms these jets is of likely stellar origin, previously expelled from…

Astrophysics · Physics 2008-10-27 V. Bosch-Ramon

The avalanche mechanism of plasma production in active galactic nuclei (AGNs) is detailed, and constraints on system parameters needed for efficient electron-positron pair cascades are explored. Whether an AGN falls within this favorable…

High Energy Astrophysical Phenomena · Physics 2026-02-03 Mikhail V. Medvedev , Andrzej A. Zdziarski

Dense populations of stars surround the nuclear regions of galaxies. In active galactic nuclei, these stars can interact with the relativistic jets launched by the supermasive black hole. In this work, we study the interaction of early-type…

High Energy Astrophysical Phenomena · Physics 2015-06-17 Anabella Araudo , Valenti Bosch-Ramon , Gustavo E. Romero
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